Gillespie, A. R.; White, G. J. and Watt, G. D.
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CO observations at 115 GHz are presented for three southern HII regions, RCW 38, RCW 122 and G 316.8-0.1. All three are shown to have large molecular clouds associated with them containing CO peaks in addition to the CO associated with the main optical-HII/radio-continuum sources These are also interpreted as sites of star formation.
|Item Type:||Journal Article|
|Copyright Holders:||1979 Royal Astronomical Society|
|Keywords:||astronomical maps; carbon monoxide; HII regions; radio astronomy; astronomical coordinates; southern hemisphere; stellar evolution|
|Academic Unit/Department:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||G. J. White|
|Date Deposited:||30 Mar 2012 09:08|
|Last Modified:||08 Oct 2016 08:19|
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